As pointed out in [1]}, in contrast to the Love number,
the tidal deformability has a wide range of values, spanning roughly
an order of magnitude over the observed mass range of neutron stars
in binary systems. The updated version of the tidal deformability
estimate for a \(1.4 \, M_{\odot }\) 
neutron star based on the gravitational-wave event GW170817 [2]}
implies that
\(70 < \Lambda _{1.4} < 580.\) 
